{"paper":{"title":"A ${\\bf 1.4}$ deg${\\bf ^2}$ blind survey for CII], CIII] and CIV at ${\\bf z\\sim0.7-1.5}$. I: nature, morphologies and equivalent widths","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Andra Stroe, David Sobral, Ivan Oteo, Jo\\~ao Calhau, Jorryt Matthee","submitted_at":"2017-03-29T18:00:02Z","abstract_excerpt":"While traditionally associated with active galactic nuclei (AGN), the properties of the CII] ($\\lambda=2326$\\,{\\AA}), CIII] ($\\lambda,\\lambda=1907,1909$\\,{\\AA}) and CIV ($\\lambda,\\lambda=1549, 1551$\\,{\\AA}) emission lines are still uncertain as large, unbiased samples of sources are scarce. We present the first blind, statistical study of CII], CIII] and CIV emitters at $z\\sim0.68,1.05,1.53$, respectively, uniformly selected down to a flux limit of $\\sim4\\times10^{-17}$ erg s$^{-1}$ cm$^{-1}$ through a narrow band survey covering an area of $\\sim1.4$ deg$^2$ over COSMOS and UDS. We detect 16 C"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.10169","kind":"arxiv","version":5},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}